Study of photon emission by electron capture during solar nuclei acceleration. 3: Photon production evaluations

Details Study of photon emission by electron capture during solar nuclei acceleration. 3: Photon production evaluations Study of photon emission by electron capture during solar nuclei acceleration. 3: Photon production evaluations

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4...26p&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 26-29 (SEE N85-34729 23-92)

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Chromosphere, Electron Capture, Particle Emission, Photons, Solar Corona, Solar Flares, Computation, Ions, Particle Acceleration, X Rays

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Lower limits of photon fluxes were evaluated from electron capture during acceleration in solar flares, because the arbitrary qc asterisk assumed in this work evolves very slow with velocity, probably much more slowly than the physical actual situation: in fact, more emission is expected toward the IR region. Nevertheless the authors claim to show that the factibility of sounding acceleration processes, charge evolution processes and physical parameters of the source itself, by the observational analysis of this kind of emissions. For instance, it would be interesting to search observationally, for the predicted flux and energy drift of Fe ions interacting with the atomic 0 and Fe of the source matter, or, even more feasible for the X-ray lines at 4.2 keV and 2.624 + 0.003 KeV from Fe and S ions in ionized Fe at T = 10 to the 7th power K respectively, the 418 + or - 2 eV and 20 + or - 4 eV lines of Fe and S in ionized Fe at 5 x 10 to the 6th power K, which are predicted from Fermi acceleration.

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